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Faylın orijinalı (2.920 × 2.920 piksel, fayl həcmi: 864 KB, MIME növü: image/jpeg)
 | Bu fayl Vikianbarda yerləşir. Açıqlama səhifəsindəki məlumatlar aşağıda göstərilib. Vikianbar azad lisenziyalı media anbarıdır. Siz də töhfə verə bilərsiniz. |
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Xülasə
| İzah |
English: NGC 7293, better known as the Helix Nebula, displays its ultraviolet glow courtesy of NASA's Galaxy Evolution Explorer (GALEX). The Helix is the nearest example of a planetary nebula, which is the eventual fate of a star, like our own Sun, as it approaches the end of its life. As it runs out of fuel, the star expels its outer envelope of gas outward to form a nebula like the Helix. The remaining core of the star is a small, hot, dense remnant known as a white dwarf. |
| Tarix | (released) |
| Mənbə | https://photojournal.jpl.nasa.gov/catalog/PIA15658 (image link) |
| Müəllif | NASA/JPL-Caltech |
This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA15658. This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing. Other languages:
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Lisenziya
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This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.) | |
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| Tarix/Vaxt | Miniatür | Ölçülər | İstifadəçi | Şərh | |
|---|---|---|---|---|---|
| hal-hazırkı | 08:17, 27 yanvar 2020 | | 2.920 × 2.920 (864 KB) | Huntster | {{Information |Description={{en|1=NGC 7293, better known as the Helix Nebula, displays its ultraviolet glow courtesy of NASA's Galaxy Evolution Explorer (GALEX). The Helix is the nearest example of a planetary nebula, which is the eventual fate of a star, like our own Sun, as it approaches the end of its life. As it runs out of fuel, the star expels its outer envelope of gas outward to form a nebula like the Helix. The remaining core of the star is a small, hot, dense remnant known as a white... |
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